Meeting contribution: Low mass stars, brown dwarfs and hot Jupiters

Details Meeting contribution: Low mass stars, brown dwarfs and hot Jupiters Meeting contribution: Low mass stars, brown dwarfs and hot Jupiters

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jbaa..117...45v&link_type=abstract

Journal of the British Astronomical Association, vol.117, no.1, p.45-46

Astronomy and Astrophysics

Astronomy

Scientific paper

Dr Viti opened with an apology that hers was not a field which could yet produce nice images; the objects she would be describing were too faint to be meaningfully imaged. Yet she would be arguing that even without images, a tremendous amount had been learnt from such objects in the past decade, and that there were exciting prospects for the future. The primary subject of this talk would be low mass stars (LMSs), defined as those stars of around half the mass of the Sun or less.

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